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Black holes quasinormal modes, Loop Quantum Gravity Immirzi parameter and nonextensive statistics.

Authors :
Abreu, Everton M.C.
Neto, Jorge Ananias
Barboza, Edésio M.
Soares, Bráulio B.
Source :
Physics Letters B. Nov2019, Vol. 798, pN.PAG-N.PAG. 1p.
Publication Year :
2019

Abstract

It is argued that, using the black hole area entropy law together with the Boltzmann-Gibbs statistical mechanics and the quasinormal modes of the black holes, it is possible to determine univocally the lowest possible value for the spin j in the context of the Loop Quantum Gravity theory which is j m i n = 1. Consequently, the value of Immirzi parameter is given by γ = ln ⁡ 3 / (2 π 2). In this paper, we have shown that if we use Tsallis microcanonical entropy rather than Boltzmann-Gibbs framework then the minimum value of the label j depends on the nonextensive q -parameter and may have values other than j m i n = 1. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
03702693
Volume :
798
Database :
Academic Search Index
Journal :
Physics Letters B
Publication Type :
Academic Journal
Accession number :
139408037
Full Text :
https://doi.org/10.1016/j.physletb.2019.135011